Variability of Hot Plasma in Solar Active Regions.

Details Variability of Hot Plasma in Solar Active Regions. Variability of Hot Plasma in Solar Active Regions.

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640712u&link_type=abstract

American Astronomical Society, AAS Meeting #216, #407.12; Bulletin of the American Astronomical Society, Vol. 41, p.861

Astronomy and Astrophysics

Astronomy

Scientific paper

The core of a solar active region is generally dominated by hot, high density, slowly evolving loops that appear to be consistent with steady heating. However, these loops are generally studied using instruments with a broad temperature response, which may mask some of the variability. Here we investigate the evolution of coronal loops emitting at temperatures above 3MK in fast scans taken with the Extreme-ultraviolet Imaging Spectrometer on board Hinode. We show evidence for short term variability at these temperatures and present the differential emission measure changes associated with them.

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